We determine the three-dimensional topography of the magnetic canopy in and around active regions by mapping the propagation behavior of high-frequency acoustic waves in the solar chromosphere
Global helioseismic oscillation modes are a window to the solar interior. They are acoustic waves tr...
The pulsation of the solar surface is caused by acoustic waves traveling in the solar interior. Thor...
We investigate deviations in the mean phase travel time of acoustic waves preceding the emergence of...
The goal of helioseismology is to provide accurate information about the Sun’s interior from the ob...
With numerical experiments we explore the feasibility of using high frequency waves for probing the ...
We show that inclined magnetic field lines at the boundaries of large-scale convective cells (superg...
Observations show the increase of high-frequency wave power near magnetic network cores and active r...
We use images of high spatial and temporal resolution, obtained using both ground- and space-based i...
We present observational evidence for the presence of MHD (magnetohydrodynamic) waves in the solar ...
We present new results of an international joint observing campaign, which was carried out in Septem...
Context. We present evidence for the conversion and transmission of wave modes on the magn...
In time-distance helioseismology the travel time of the acoustic waves between different points on t...
Aims: We analyse numerically the propagation and dispersion of acoustic waves in the solar-like sub-...
Abstract. We analyze oscillations in the solar atmosphere using image sequences from the Transition ...
© The Author(s) 2008. This article is published with open access at Springerlink.com Abstract Variou...
Global helioseismic oscillation modes are a window to the solar interior. They are acoustic waves tr...
The pulsation of the solar surface is caused by acoustic waves traveling in the solar interior. Thor...
We investigate deviations in the mean phase travel time of acoustic waves preceding the emergence of...
The goal of helioseismology is to provide accurate information about the Sun’s interior from the ob...
With numerical experiments we explore the feasibility of using high frequency waves for probing the ...
We show that inclined magnetic field lines at the boundaries of large-scale convective cells (superg...
Observations show the increase of high-frequency wave power near magnetic network cores and active r...
We use images of high spatial and temporal resolution, obtained using both ground- and space-based i...
We present observational evidence for the presence of MHD (magnetohydrodynamic) waves in the solar ...
We present new results of an international joint observing campaign, which was carried out in Septem...
Context. We present evidence for the conversion and transmission of wave modes on the magn...
In time-distance helioseismology the travel time of the acoustic waves between different points on t...
Aims: We analyse numerically the propagation and dispersion of acoustic waves in the solar-like sub-...
Abstract. We analyze oscillations in the solar atmosphere using image sequences from the Transition ...
© The Author(s) 2008. This article is published with open access at Springerlink.com Abstract Variou...
Global helioseismic oscillation modes are a window to the solar interior. They are acoustic waves tr...
The pulsation of the solar surface is caused by acoustic waves traveling in the solar interior. Thor...
We investigate deviations in the mean phase travel time of acoustic waves preceding the emergence of...
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